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Liam Krauss
Movie   ID   Title
SeaWiFS Biosphere data symbolizing the heartbeat of our planet.   2395   Pulse of the Planet
Density and magnetic flux surfaces from a simulation of magnetic flux in the solar atmosphere undergoing velocity perturbations. This run has a vertical scale height of 6.8 million meters.   1418   High Resolution 2-D Numerical Simulation of Emergence of Magnetic Flux Through the Solar Atmosphere
Various quantities from a simulation of magnetic flux in the solar atmosphere undergoing velocity perturbations. This run has a vertical scale height of 6.8 million meters.   1417   High Resolution 2-D Numerical Simulation of Emergence of Magnetic Flux Through the Solar Atmosphere
Various quantities from a simulation of magnetic flux in the solar atmosphere undergoing velocity perturbations. This run has a vertical scale height of 4.8 million meters.   1416   High Resolution 2-D Numerical Simulation of Emergence of Magnetic Flux Through the Solar Atmosphere
Magnetic field lines superimposed over density are compared for a 2D global hybrid simulation and a magnetohydrodynamic model of the solar wind-magnetosphere interaction   1393   Global Hybrid Versus MHD Modeling of the Magnetosphere: Density and Magnetic Field
The entire narrated Images video made for Supercomputing 97   251   Images of Earth and Space: SC97 Edition
This image represents a one month sample (October 1983) of composite images from cloud cover data collected from a suite of U.S., European, and Japanese geostationary satellites and U.S. polar orbiting meteorological satellites.   155   The HoloGlobe Project (Version 3)
An interactive exploration of a computational model of Hurricane Florence using an immersive environment controlled by a boom, with an inset of the boom operator.   122   Hurricane Florence Mesoscale Simulation Results Using Virtual Reality
Contour lines of the z-component of the magnetic potential are compared for a 2D global hybrid simulation and a magnetohydrodynamic model of the solar wind-magnetosphere interaction   117   Global Hybrid Versus MHD Modeling of the Magnetosphere: Magnetic Potential
Narrated Hologlobe (version 2)   116   The HoloGlobe Project (Version 2)
A animation of the evolution of the density gradient and velocities in the solar atmosphere model. The three velocities shown are the velocity normalized to the fast magnetosonic speed and the velocities parallel and perpendicular to the magnetic field. Mach number contours are shown in green.   115   Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density Gradient and Velocities
A animation of the evolution of the density gradient, the magnetic field, and the mach number in the solar atmosphere model. Magnetic field contours are shown in magenta and mach number contours are shown in green.   114   Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density Gradient, Magnetic Field, and Mach Number
A animation of the evolution of the density, the magnetic field, and the mach number in the solar atmosphere model. Magnetic field contours are shown in black and mach number contours are shown in green.   113   Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density, Magnetic Field, and Mach Number
A animation of the evolution of the density gradient in the solar atmosphere model   112   Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density Gradient
A animation of the evolution of the density in the solar atmosphere model   111   Numerical Simulation of Magnetic Flux Emerging Through a Model Solar Atmosphere: Density
Density and magnetic flux surfaces from a simulation of magnetic flux in the solar atmosphere undergoing velocity perturbations. This run has a vertical scale height of 4.8 million meters.   107   High Resolution 2-D Numerical Simulation of Emergence of Magnetic Flux Through the Solar Atmosphere
Hologlobe (version 1)   96   The HoloGlobe Project (Version 1)
A comparison of energetic electron fluxes (> 0.4 MeV) over the North Pole from the PET P1 solid state detector during the period 7-19-1993 through 8-6-1994 with soft X-ray images from Yohkoh   90   SAMPEX - Yohkoh: Solar Modification of Relativistic Electrons in the Earth's Radiation Belts
This animation presents correlated measurements and model data for an impact of a magnetic cloud originating from the Sun on the Earths magnetosphere on October 18-20, 1995.   88   Magnetic Cloud Event: October 18-20, 1995
Magnetic field lines superimposed over density for a 2D simulation of the solar wind-magnetosphere interaction   87   2-D Unstructured Mesh Particle-MHD Solar Wind Flow Over the Earth:Density and Magnetic Field
Contour lines of the z-component of the magnetic potential for a 2D simulation of the solar wind-magnetosphere interaction   86   2-D Unstructured Mesh Particle-MHD Solar Wind Flow Over the Earth: Magnetic Potential
Video of an operator using a boom to control an immersive application   83   VR Operator
An interactive exploration of a computational model of Hurricane Florence using an immersive environment controlled by a boom   82   Hurricane Florence
An interactive exploration of a computational model of Hurricane Florence using an immersive environment controlled by a boom, with an inset of the boom operator.   81   Hurricane Florence with Inset of VR Operator


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